activity
19972026
most citedWater in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

262 citations · 10.6k across the 258 of their papers we have counts for

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Showing 2011Show all

7 papers · 1 filter

astro-ph.SR2011★ 46 cited

The Herschel HIFI water line survey in the low-mass proto-stellar outflow L1448

G. Santangelo, B. Nisini, T. Giannini +8

As part of the WISH (Water In Star-forming regions with Herschel) key project, we report on the observations of several ortho- and para-H2O lines performed with the HIFI instrument…

astro-ph.GA2011★ 36 cited

Water emission from the chemically rich outflow L1157

M. Vasta, C. Codella, A. Lorenzani +7

In the framework of the Herschel-WISH key program, several ortho-H2O and para-H2O emission lines, in the frequency range from 500 to 1700 GHz, were observed with the HIFI instrumen…

astro-ph.GA2011★ 28 cited

First detection of Hydrogen Chloride towards protostellar shocks

C. Codella, C. Ceccarelli, S. Bottinelli +8

We present the first detection of hydrogen chlorine in a protostellar shock, by observing the fundamental transition at 626 GHz with the Herschel HIFI spectrometer. We detected two…

astro-ph.GA2011★ 83 cited

L1157-B1: Water and ammonia as diagnostics of shock temperature

S. Viti, I. Jimenez-Serra, J. A. Yates +5

We investigate the origin and nature of the profiles of water and ammonia observ ed toward the L1157-B1 clump as part of the HIFI CHESS survey (Ceccarelli et al. 2010) using a new…

astro-ph.GA2011★ 38 cited

Molecular outflows and hot molecular core in G24.78+0.08 at sub-arcsecond angular resolution

M. T. Beltran, R. Cesaroni, Q. Zhang +5

Context. This study is part of a large project to study the physics of accretion and molecular outflows towards a selected sample of high-mass star-forming regions that show eviden…

astro-ph.SR2011★ 46 cited

On the kinematics of massive star forming regions: the case of IRAS 17233-3606

S. Leurini, C. Codella, L. Zapata +3

Direct observations of accretion disks around high-mass young stellar objects would help to discriminate between different models of formation of massive stars. However, given the…